We present results of the large-scale structure analysis
from the largest of the Spitzer Legacy programs, the Spitzer
Wide-Area Infrared Extragalactic Survey (SWIRE). As the
widest-area survey using Spitzer covering 50 square degrees,
SWIRE provides unprecedented grand view of the galaxies and
structures in infrared universe from 3.6 to 160 microns,
tracing their evolution to a redshift of 2.5 and beyond. We
use a variety of techniques to analyze the spatial
distribution of SWIRE galaxies from mid- to far-infrared
wavelengths. We discuss our analysis and implications of our
results on underlying structures and evolution models from
the infrared view.

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for comments about the abstract:
fan@ipac.caltech.edu